Abstract
Appleton1 and Hey2 have directed attention to the fact that radio- frequency energy, with some of the characteristics of random ‘noise’, is emitted with greatly increased intensity from the sun under the conditions of violent disturbance associated with a large sunspot. These observations were confined mainly to the region of frequencies near 60 Mc./s.
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Reference
Appleton, Nature, 158, 534 (1945).
Hey, Nature, 157, 47 (1946).
Pawsey, Payne-Scott and McCready, Nature, 157, 158 (1946).
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© 1946 Macmillan Journals Ltd.
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Ryle, M., Vonberg, D.D. (1946). Solar Radiation on 175 Mc./s.. In: Classics in Radio Astronomy. Studies in the History of Modern Science, vol 10. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7752-5_18
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DOI: https://doi.org/10.1007/978-94-009-7752-5_18
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